Simple models for magnetic flux tubes

Details Simple models for magnetic flux tubes Simple models for magnetic flux tubes

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...87...65s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 87, Aug. 1983, p. 65-75.

Physics

18

Magnetic Flux, Photosphere, Solar Magnetic Field, Bessel Functions, Field Theory (Physics), Stellar Models, Step Functions

Scientific paper

Known potential field solutions can be used to model the structure of magnetic fields in the solar photosphere. Several two-dimensional and axisymmetric solutions are compared. In the most satisfactory model the vertical component of the field is prescribed on a horizontal plane so as to be uniform within a finite disc and zero outside it. The resulting flux distribution provides a good description of small scale intergranular magnetic fields and of the observed field structure in a pore, but is inadequate for sunspots.

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